Tracing Cosmic Evolution:
From the CMB to the Web, the CGM, and Galactic Disks





What if the galaxy had formed here instead?




What if the galaxy had formed here instead?


or here?
The “splicing” technique


- Generate ICs
- Integrate (\(N\)-body)
- Select region of interest
- Trace back to ICs
- “Splice” the region
- Integrate again

\(t\)
Splicing: equivalent of constraining density field at all points in region
\(\longleftarrow 50\,\mathrm{Mpc} \longrightarrow\)
Splicing in 1D


Splicing in 1D


Most likely field \(f\) with
- same value in spliced region (\(a\)),
- as close as possible outside (\(b\))
Mathematically, \({\color{green}f}\) is the unique solution that satisfies:
- \( {\color{green}f(x)}= {\color{blue}a(x)},\qquad\qquad\qquad\forall x \in\Gamma\)
- minimizes \[\mathcal{Q} = ({\color{red}b}-{\color{green}f})^\dagger\mathbf{C}^{-1}({\color{red}b}-{\color{green}f}),\quad \forall x \not\in \Gamma \]



-

-
The causal origin of DM halo concentration


\(M^{(1)}_{200\mathrm{c}}, c^{(1)}_\mathrm{NFW}, \dots\)


\(M^{(2)}_{200\mathrm{c}}, c^{(2)}_\mathrm{NFW}, \dots\)


\(M^{(\dots)}_{200\mathrm{c}}, c^{(\dots)}_\mathrm{NFW}, \dots\)


\(M^{(10)}_{200\mathrm{c}}, c^{(10)}_\mathrm{NFW}, \dots\)
Same halo in 10× different environments
Repeat experiment for 7 halos (70 realisations in total)
Same halo in 10× different environments
Repeat experiment for 7 halos (70 realisations in total)


\(M^{(1)}_{200\mathrm{c}}, c^{(1)}_\mathrm{NFW}, \dots\)


\(M^{(2)}_{200\mathrm{c}}, c^{(2)}_\mathrm{NFW}, \dots\)


\(M^{(\dots)}_{200\mathrm{c}}, c^{(\dots)}_\mathrm{NFW}, \dots\)


\(M^{(10)}_{200\mathrm{c}}, c^{(10)}_\mathrm{NFW}, \dots\)
The causal origin of DM halo concentration
Same halo in 10× different environments
Repeat experiment for 7 halos (70 realisations in total)


\(M^{(1)}_{200\mathrm{c}}, c^{(1)}_\mathrm{NFW}, \dots\)


\(M^{(2)}_{200\mathrm{c}}, c^{(2)}_\mathrm{NFW}, \dots\)


\(M^{(\dots)}_{200\mathrm{c}}, c^{(\dots)}_\mathrm{NFW}, \dots\)


\(M^{(10)}_{200\mathrm{c}}, c^{(10)}_\mathrm{NFW}, \dots\)

The causal origin of DM halo concentration
50% of population



\(\log\left|\dfrac{{\color{blue}\rho_\mathrm{i}} - \color{red}\rho_\mathrm{i}}{\sigma_\rho}\right|\)
\(\log\left|\dfrac{{\color{blue}v_\mathrm{i}} - \color{red}v_\mathrm{i}}{\sigma_v}\right|\)

Issue : splicing the density does not fix the velocity & tides




Issue : splicing the density does not fix the velocity & tides
Solution: splice the potential
\(\log\left|\dfrac{{\color{blue}\rho_\mathrm{i}} - \color{red}\rho_\mathrm{i}}{\sigma_\rho}\right|\)
\(\log\left|\dfrac{{\color{blue}v_\mathrm{i}} - \color{red}v_\mathrm{i}}{\sigma_v}\right|\)
Remember \(\nabla^2\phi = 4\pi G\rho\) so
\[\rho_n\propto\frac{\phi_{n+1}-2\phi_n+\phi_{n-1}}{\Delta x^2}\]
\[v_n\propto\frac{\phi_{n+1}-\phi_{n-1}}{2\Delta x}\]
DM angular momentum

\(z=0\)
\( z = 100\)

\(z=0\)
\( z = 100\)
[White 84]
DM angular momentum

\(z=0\)
\( z = 100\)
[Genetic modifications: Roth+16, see also Rey&Pontzen 18, Stopyra+20]


DM angular momentum





Time
Angular
momentum
DM angular momentum
✅ AM of fixed DM regions responds ~linearly (so is not chaotic!)
However, particle membership hence DM halo does not
Angular
momentum
Time
DM angular momentum
Copy of Tracing Cosmic Evolution: From the CMB to the Web, the CGM, and Galactic Disks @ Korea
By Corentin Cadiou
Copy of Tracing Cosmic Evolution: From the CMB to the Web, the CGM, and Galactic Disks @ Korea
IAP Seminar
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